! Started logfile: J0413-0615_S_2004_05_27_yyk_uvs.log on Wed Dec  7 01:03:03 2005
obs J0413-0615_S_2004_05_27_yyk_uve.fits
! Reading UV FITS file: J0413-0615_S_2004_05_27_yyk_uve.fits
! AN table 1: 22 integrations on 45 of 45 possible baselines.
! Apparent sampling: 0.467677 visibilities/baseline/integration-bin.
! *** This seems a bit low - see "help observe" on the binwid argument.
! Found source: J0413-0615
! 
! There are 4 IFs, and a total of 4 channels:
! 
!  IF  Channel    Frequency  Freq offset  Number of   Overall IF
!       origin    at origin  per channel   channels    bandwidth
!  ------------------------------------------------------------- (Hz)
!  01        1  2.23697e+09        8e+06          1        8e+06
!  02        2  2.26697e+09        8e+06          1        8e+06
!  03        3  2.35697e+09        8e+06          1        8e+06
!  04        4  2.37697e+09        8e+06          1        8e+06
! 
! Polarization(s): RR
! 
! Read 1388 lines of history.
! 
! Reading 1852 visibilities.
select I
! Polarization I is unavailable.
! Selecting polarization: RR,  channels: 1..4
! Reading IF 1 channels: 1..1
! Reading IF 2 channels: 2..2
! Reading IF 3 channels: 3..3
! Reading IF 4 channels: 4..4
![@muppet J0413-0615_S_2004_05_27_yyk]
integer clean_niter
clean_niter = 100
float clean_gain
clean_gain = 0.04
float dynam
dynam = 6.0
float amp_soltime1
amp_soltime1 = 10
float amp_soltime2
amp_soltime2 = 1
float phase_soltime1
phase_soltime1=10
float phase_soltime2
phase_soltime2=0.5
float phase_soltime
phase_soltime=phase_soltime1
float ampcor_selflim
ampcor_selflim=1.20
float thresh
thresh = 0.10
float win_mult
win_mult = 1.8
float time_av
time_av = 30
float old_peak
float new_peak
float flux_cutoff
mapsize field_size, field_cell
! Map grid = 256x256 pixels with 1.00x1.00 milli-arcsec cellsize.
phase_soltime=phase_soltime1
print "uvstat(rms)=",uvstat(rms),"Jy"
! uvstat(rms)= 0.105996 Jy 
startmod ,phase_soltime
! Applying default point source starting model.
! Performing phase self-cal over 10 minute time intervals
! Adding 1 model components to the UV plane model.
! The established model now contains 1 components and 1 Jy
! 
! Correcting IF 1.
!  A total of 144 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 2.
!  A total of 88 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 3.
!  A total of 87 telescope corrections were flagged in sub-array 1.
! 
! Correcting IF 4.
!  A total of 101 telescope corrections were flagged in sub-array 1.
! 
! Fit before self-cal, rms=0.950497Jy  sigma=15.362146
! Fit after  self-cal, rms=0.949476Jy  sigma=15.347080
! clrmod: Cleared the established, tentative and continuum models.
! Redundant starting model cleared.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=7.573 mas, bmaj=13.34 mas, bpa=2.23 degrees
! Estimated noise=1.84627 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! Added new window around map position (0, 0).
! clean: niter=100  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.0484073 Jy
! Component: 100  -  total flux cleaned = 0.0531543 Jy
! Total flux subtracted in 100 components = 0.0531543 Jy
! Clean residual min=-0.006600 max=0.008065 Jy/beam
! Clean residual mean=0.000037 rms=0.002266 Jy/beam
! Combined flux in latest and established models = 0.0531543 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 13 components and 0.0531543 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.090387Jy  sigma=1.092414
! Fit after  self-cal, rms=0.090068Jy  sigma=1.087403
! Inverting map 
print "************** FINISHED UNIFORM WEIGHTING CLEAN **************"
! ************** FINISHED UNIFORM WEIGHTING CLEAN ************** 
! 
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
win_mult = win_mult * 1.6
clean_niter = clean_niter * 2
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=8.532 mas, bmaj=14.31 mas, bpa=4.753 degrees
! Estimated noise=1.30739 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00629196 Jy
! Component: 100  -  total flux cleaned = 0.00871468 Jy
! Component: 150  -  total flux cleaned = 0.00925113 Jy
! Component: 200  -  total flux cleaned = 0.00929683 Jy
! Total flux subtracted in 200 components = 0.00929683 Jy
! Clean residual min=-0.004483 max=0.004748 Jy/beam
! Clean residual mean=0.000062 rms=0.001333 Jy/beam
! Combined flux in latest and established models = 0.0624511 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 22 model components to the UV plane model.
! The established model now contains 31 components and 0.0624511 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.090053Jy  sigma=1.080910
! Fit after  self-cal, rms=0.090057Jy  sigma=1.080847
! Inverting map 
print "************** FINISHED NATURAL WEIGHTING CLEAN **************"
! ************** FINISHED NATURAL WEIGHTING CLEAN ************** 
! 
selflims ampcor_selflim
! Selfcal amplitude corrections will be limited to 0.833333 -> 1.2.
! Selfcal phase corrections will not be limited.
gscale
! Performing overall amplitude self-cal
! 
! Correcting IF 1.
!  Amplitude normalization factor in sub-array 1: 0.991239
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.08     HN        1.00*    KP        0.86     
!   LA        0.96     MK        1.00*    NL        1.05     OV        1.16     
!   PT        0.98     SC        1.00*    
! 
! 
! Correcting IF 2.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Correcting IF 3.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1
!  Telescope amplitude corrections in sub-array 1:
!   BR        1.00*    FD        1.00*    HN        1.00*    KP        1.00*    
!   LA        1.00*    MK        1.00*    NL        1.00*    OV        1.00*    
!   PT        1.00*    SC        1.00*    
! 
! 
! Correcting IF 4.
!  A total of 3 telescope corrections were flagged in sub-array 1.
!  Amplitude normalization factor in sub-array 1: 1.07301
!  Telescope amplitude corrections in sub-array 1:
!   BR        0.87     FD        0.90     HN        0.85     KP        1.01     
!   LA        1.00*    MK        1.00*    NL        0.86     OV        0.97     
!   PT        0.86     SC        1.00*    
! 
! 
! Fit before self-cal, rms=0.090057Jy  sigma=1.080847
! Fit after  self-cal, rms=0.087917Jy  sigma=1.077196
selfcal false, false, phase_soltime
! Performing phase self-cal over 10 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087917Jy  sigma=1.077196
! Fit after  self-cal, rms=0.087943Jy  sigma=1.077010
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=8.518 mas, bmaj=14.3 mas, bpa=4.567 degrees
! Estimated noise=1.28733 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = -0.00129205 Jy
! Component: 100  -  total flux cleaned = -0.00140928 Jy
! Component: 150  -  total flux cleaned = -0.00147796 Jy
! Component: 200  -  total flux cleaned = -0.00153723 Jy
! Total flux subtracted in 200 components = -0.00153723 Jy
! Clean residual min=-0.004764 max=0.004851 Jy/beam
! Clean residual mean=0.000065 rms=0.001318 Jy/beam
! Combined flux in latest and established models = 0.0609138 Jy
! Performing phase self-cal over 10 minute time intervals
! Adding 10 model components to the UV plane model.
! The established model now contains 38 components and 0.0609138 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087857Jy  sigma=1.076360
! Fit after  self-cal, rms=0.087856Jy  sigma=1.076291
! Inverting map 
print "************** FINISHED AMPLITUDE GSCALE SELF-CAL **************"
! ************** FINISHED AMPLITUDE GSCALE SELF-CAL ************** 
! 
phase_soltime=phase_soltime2
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.087856Jy  sigma=1.076291
! Fit after  self-cal, rms=0.080312Jy  sigma=0.966504
dynam = dynam - 0.5
flux_cutoff = imstat(rms) * dynam
! Inverting map 
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00616809 Jy
! Component: 100  -  total flux cleaned = 0.00652575 Jy
! Component: 150  -  total flux cleaned = 0.00657176 Jy
! Component: 200  -  total flux cleaned = 0.00650172 Jy
! Total flux subtracted in 200 components = 0.00650172 Jy
! Clean residual min=-0.003606 max=0.004033 Jy/beam
! Clean residual mean=0.000044 rms=0.001120 Jy/beam
! Combined flux in latest and established models = 0.0674156 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 13 model components to the UV plane model.
! The established model now contains 47 components and 0.0674156 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.079881Jy  sigma=0.958572
! Fit after  self-cal, rms=0.079023Jy  sigma=0.948195
! Inverting map 
print "*** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime ***"
! *** FINISHED NATURAL WEIGHTING CLEAN with shorter phase_soltime *** 
! 
dynam = dynam - 0.25
restore
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 8.518 x 14.3 at 4.567 degrees (North through East)
! Clean map  min=-0.0034573  max=0.066119 Jy/beam
if(peak(flux) > thresh)
  selfcal true, true, amp_soltime1
  selfcal false, false, phase_soltime
  flux_cutoff = imstat(rms) * dynam
  repeat
    if (peak(flux) > flux_cutoff) peakwin win_mult
    clean clean_niter,clean_gain
    flux_cutoff = imstat(rms) * dynam
    selfcal false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  selfcal true, true, amp_soltime2
  selfcal false, false, phase_soltime
  flux_cutoff = imstat(rms) * dynam
  repeat
    if (peak(flux) > flux_cutoff) peakwin win_mult
    clean clean_niter,clean_gain
    flux_cutoff = imstat(rms) * dynam
    selfcal false,false,phase_soltime
    new_peak = peak(flux)
    until(new_peak<=flux_cutoff)
  print "************** FINISHED AMPLITUDE SELF-CAL **************"
  end if
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths.
win_mult = win_mult * 1.4
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=9.929 mas, bmaj=15.53 mas, bpa=4.165 degrees
! Estimated noise=1.32567 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  selfcal false,false,phase_soltime
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000223621 Jy
! Component: 100  -  total flux cleaned = 0.000115089 Jy
! Component: 150  -  total flux cleaned = 4.25233e-05 Jy
! Component: 200  -  total flux cleaned = -1.41967e-06 Jy
! Total flux subtracted in 200 components = -1.41967e-06 Jy
! Clean residual min=-0.003200 max=0.003894 Jy/beam
! Clean residual mean=0.000059 rms=0.001139 Jy/beam
! Combined flux in latest and established models = 0.0674141 Jy
! Performing phase self-cal over 0.5 minute time intervals
! Adding 14 model components to the UV plane model.
! The established model now contains 54 components and 0.0674141 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078983Jy  sigma=0.947877
! Fit after  self-cal, rms=0.078675Jy  sigma=0.945976
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
win_mult = win_mult / 1.4
print "************** FINISHED TAPERING SELF-CAL CLEAN **************"
! ************** FINISHED TAPERING SELF-CAL CLEAN ************** 
! 
print "************** CLEARING MODEL AND STARTING OVER **********"
! ************** CLEARING MODEL AND STARTING OVER ********** 
clrmod true,true,true
! clrmod: Cleared the established, tentative and continuum models.
uvw 2,-1
! Uniform weighting binwidth: 2 (pixels).
! Gridding weights will be scaled by errors raised to the power -1.
! Radial weighting is not currently selected.
clean clean_niter, clean_gain
! Inverting map and beam 
! Estimated beam: bmin=7.56 mas, bmaj=13.33 mas, bpa=1.987 degrees
! Estimated noise=1.8192 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.057683 Jy
! Component: 100  -  total flux cleaned = 0.0620014 Jy
! Component: 150  -  total flux cleaned = 0.0623186 Jy
! Component: 200  -  total flux cleaned = 0.0611766 Jy
! Total flux subtracted in 200 components = 0.0611766 Jy
! Clean residual min=-0.005421 max=0.005451 Jy/beam
! Clean residual mean=0.000024 rms=0.001729 Jy/beam
! Combined flux in latest and established models = 0.0611767 Jy
uvw 0,-2
! Uniform weighting is not currently selected.
! Gridding weights will be scaled by errors raised to the power -2.
! Radial weighting is not currently selected.
flux_cutoff = imstat(rms) * dynam
! Adding 19 model components to the UV plane model.
! The established model now contains 19 components and 0.0611767 Jy
! Inverting map and beam 
! Estimated beam: bmin=8.518 mas, bmaj=14.3 mas, bpa=4.567 degrees
! Estimated noise=1.28733 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.00390287 Jy
! Component: 100  -  total flux cleaned = 0.00492987 Jy
! Component: 150  -  total flux cleaned = 0.00519093 Jy
! Component: 200  -  total flux cleaned = 0.00536588 Jy
! Total flux subtracted in 200 components = 0.00536588 Jy
! Clean residual min=-0.003850 max=0.004034 Jy/beam
! Clean residual mean=0.000049 rms=0.001157 Jy/beam
! Combined flux in latest and established models = 0.0665425 Jy
! Adding 22 model components to the UV plane model.
! The established model now contains 40 components and 0.0665425 Jy
! Inverting map 
uvtaper 0.3,taper_size
! Gaussian taper: value 0.3 at UV radius = 20 mega-wavelengths.
flux_cutoff = imstat(rms) * dynam
! Inverting map and beam 
! Estimated beam: bmin=9.929 mas, bmaj=15.53 mas, bpa=4.165 degrees
! Estimated noise=1.32567 mJy/beam.
repeat
  if (peak(flux) > flux_cutoff) peakwin win_mult
  clean clean_niter,clean_gain
  flux_cutoff = imstat(rms) * dynam
  keep
  new_peak = peak(flux)
  until(new_peak<=flux_cutoff)
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 0.000308274 Jy
! Component: 100  -  total flux cleaned = 0.000365282 Jy
! Component: 150  -  total flux cleaned = 0.00044106 Jy
! Component: 200  -  total flux cleaned = 0.000485469 Jy
! Total flux subtracted in 200 components = 0.000485469 Jy
! Clean residual min=-0.003282 max=0.003969 Jy/beam
! Clean residual mean=0.000061 rms=0.001166 Jy/beam
! Combined flux in latest and established models = 0.067028 Jy
! Adding 13 model components to the UV plane model.
! The established model now contains 49 components and 0.067028 Jy
! Inverting map 
uvtaper 0,0
! No UV-taper is currently set.
clean
! Inverting map and beam 
! Estimated beam: bmin=8.518 mas, bmaj=14.3 mas, bpa=4.567 degrees
! Estimated noise=1.28733 mJy/beam.
! clean: niter=200  gain=0.04  cutoff=0
! Component: 050  -  total flux cleaned = 4.70079e-05 Jy
! Component: 100  -  total flux cleaned = 9.7951e-05 Jy
! Component: 150  -  total flux cleaned = 0.0001457 Jy
! Component: 200  -  total flux cleaned = 0.000145461 Jy
! Total flux subtracted in 200 components = 0.000145461 Jy
! Clean residual min=-0.003698 max=0.003831 Jy/beam
! Clean residual mean=0.000047 rms=0.001119 Jy/beam
! Combined flux in latest and established models = 0.0671735 Jy
selfcal false, false, phase_soltime
! Performing phase self-cal over 0.5 minute time intervals
! Adding 12 model components to the UV plane model.
! The established model now contains 55 components and 0.0671735 Jy
! 
! Correcting IF 1.
! 
! Correcting IF 2.
! 
! Correcting IF 3.
! 
! Correcting IF 4.
! 
! Fit before self-cal, rms=0.078703Jy  sigma=0.945956
! Fit after  self-cal, rms=0.078596Jy  sigma=0.945528
wmodel J0413-0615_S_2004_05_27_yyk\_map.mod
! Writing 55 model components to file: J0413-0615_S_2004_05_27_yyk_map.mod
wobs J0413-0615_S_2004_05_27_yyk\_uvs.fits
! Writing UV FITS file: J0413-0615_S_2004_05_27_yyk_uvs.fits
wwins J0413-0615_S_2004_05_27_yyk\_map.win
! wwins: Wrote 1 windows to J0413-0615_S_2004_05_27_yyk_map.win
x = (field_size-8) * field_cell / 4
addwin -x,x,-x,x
clean (field_size*4),0.01
! Inverting map 
! clean: niter=1024  gain=0.01  cutoff=0
! Component: 050  -  total flux cleaned = 0.000409707 Jy
! Component: 100  -  total flux cleaned = 0.000962275 Jy
! Component: 150  -  total flux cleaned = 0.00131302 Jy
! Component: 200  -  total flux cleaned = 0.00130979 Jy
! Component: 250  -  total flux cleaned = 0.00126532 Jy
! Component: 300  -  total flux cleaned = 0.00122585 Jy
! Component: 350  -  total flux cleaned = 0.00138439 Jy
! Component: 400  -  total flux cleaned = 0.0014959 Jy
! Component: 450  -  total flux cleaned = 0.0015323 Jy
! Component: 500  -  total flux cleaned = 0.00156715 Jy
! Component: 550  -  total flux cleaned = 0.00163552 Jy
! Component: 600  -  total flux cleaned = 0.0015354 Jy
! Component: 650  -  total flux cleaned = 0.0015677 Jy
! Component: 700  -  total flux cleaned = 0.0016312 Jy
! Component: 750  -  total flux cleaned = 0.0016932 Jy
! Component: 800  -  total flux cleaned = 0.00175442 Jy
! Component: 850  -  total flux cleaned = 0.00187387 Jy
! Component: 900  -  total flux cleaned = 0.00190337 Jy
! Component: 950  -  total flux cleaned = 0.00196125 Jy
! Component: 1000  -  total flux cleaned = 0.00201831 Jy
! Total flux subtracted in 1024 components = 0.00210192 Jy
! Clean residual min=-0.001389 max=0.001943 Jy/beam
! Clean residual mean=0.000038 rms=0.000645 Jy/beam
! Combined flux in latest and established models = 0.0692754 Jy
keep
! Adding 65 model components to the UV plane model.
! The established model now contains 120 components and 0.0692754 Jy
![Exited script file: muppet]
wmap "J0413-0615_S_2004_05_27_yyk\_map.fits"
! Inverting map 
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 8.518 x 14.3 at 4.567 degrees (North through East)
! Clean map  min=-0.0030751  max=0.066694 Jy/beam
! Writing clean map to FITS file: J0413-0615_S_2004_05_27_yyk_map.fits
float peak_flux
peak_flux = peak(flux,max)
print "The peak flux is",peak_flux
! The peak flux is 0.0666938 
invert
! Inverting map 
float image_rms
image_rms = imstat(rms)
print "The final image rms is",image_rms
! The final image rms is 0.000651293 
device "J0413-0615_S_2004_05_27_yyk\_map.eps/VPS"
! Attempting to open device: 'J0413-0615_S_2004_05_27_yyk_map.eps/VPS'
loglevs 1*100*3*image_rms/peak_flux
! The new contour levels are:
!  -2.92963 2.92963 5.85925 11.7185 23.437 46.874 93.748
print "clev=",int(1*3*image_rms*10000)/10000
! clev= 0.0019 
print "peak=",int(peak_flux*1000)/1000
! peak= 0.066 
mapcolor none
! Mapplot colormap: none, contrast: 1 brightness: 0.5.
mapplot cln
! restore: Substituting estimate of restoring beam from last 'invert'.
! Restoring with beam: 8.518 x 14.3 at 4.567 degrees (North through East)
! Clean map  min=-0.0030751  max=0.066694 Jy/beam
mapcolor color, 0.9
! Mapplot colormap: rainbow, contrast: 0.9 brightness: 0.5.
device "J0413-0615_S_2004_05_27_yyk\_map.gif/gif"
! Attempting to open device: 'J0413-0615_S_2004_05_27_yyk_map.gif/gif'
mapplot cln
quit
! Quitting program
! Log file J0413-0615_S_2004_05_27_yyk_uvs.log closed on Wed Dec  7 01:03:04 2005